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Related papers: Morphologies of Wolf-Rayet Planetary Nebulae based…

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We present new HST/WFC3-IR narrowband [Fe II] images of protostellar jets in the Carina Nebula. Combined with 5 previously published sources, we have a sample of 18 jets and 2 HH objects. All of the jets we targeted with WFC3 show bright…

Solar and Stellar Astrophysics · Physics 2016-09-21 Megan Reiter , Nathan Smith , John Bally

NGC 7582 is an SB(s)ab galaxy which displays evidences of simultaneous nuclear activity and star formation in its centre. Previous optical observations revealed, besides the H II regions, an ionization cone and a gas disc in its central…

Astrophysics of Galaxies · Physics 2017-11-15 T. V. Ricci , J. E. Steiner , D. May , A. Garcia-Rissmann , R. B. Menezes

We have studied the planetary nebula (PN) NGC 6572 through 3D morpho-kinematic and photoionization modelling. The 3D morphology is reconstructed from the Hubble Space Telescope images in different narrow band filters and position-velocity…

Solar and Stellar Astrophysics · Physics 2023-07-05 Rahul Bandyopadhyay , Ramkrishna Das , Mudumba Parthasarathy , Subhajit Kar

We present a set of four Gemini-North GMOS/IFU observations of the central disturbed regions of the dwarf irregular starburst galaxy NGC 1569, surrounding the well-known super star clusters A and B. This continues on directly from a…

Astrophysics · Physics 2009-11-13 M. S. Westmoquette , L. J. Smith , J. S. Gallagher , K. M. Exter

Stars like the Sun expel their outer layers and form planetary nebulae (PNe) as they evolve into white dwarfs. PNe exhibit diverse morphologies, the origins of which are not fully understood. PNe with OH (OHPNe) and H$_{2}$O (H$_{2}$OPNe)…

(Abridged) In this second paper of the series, we present the results from optical Gemini-North GMOS-IFU and WIYN DensePak IFU spectroscopic observations of the starburst and inner wind zones of M82, with a focus on the state of the T~10^4…

Cosmology and Nongalactic Astrophysics · Physics 2015-05-13 M. S. Westmoquette , J. S. Gallagher , L. J. Smith , G. Trancho , N. Bastian , I. S. Konstantopoulos

We report a multi-wavelength study of four new planetary nebula (PN) candidates selected from the INT/WFC Photometric Ha Survey of the Northern Galactic Plane (IPHAS) and Deep Sky Hunter (DSH) catalogues. We present mid-resolution optical…

Solar and Stellar Astrophysics · Physics 2015-06-18 Chih-Hao Hsia , Yong Zhang

We report optical integral-field spectroscopy in the field of one of the most luminous quasars in the $z < 1$ Universe, PKS0454-22, with the Multi-Unit Spectroscopic Explorer. These data enable the discovery of three large ionized nebulae…

Astrophysics of Galaxies · Physics 2025-02-20 Jakob M. Helton , Sean D. Johnson , Jenny E. Greene , Hsiao-Wen Chen

Hu\,1-2 is a planetary nebula that contains an isolated knot located northwestern of the main nebula, which could be related to a collimated outflow. We present a subsarcsecond H$\alpha$+[N\,{\sc ii}] image and a high-resolution, long-slit…

Astrophysics of Galaxies · Physics 2015-06-03 L. F. Miranda , M. Blanco , M. A. Guerrero , A. Riera

Wolf-Rayet star's winds can be so dense and so optically thick that the photosphere appears in the highly supersonic part of the outflow, veiling the underlying subsonic part of the star, and leaving the initial acceleration of the wind…

Solar and Stellar Astrophysics · Physics 2018-07-04 Luca Grassitelli , Norbert Langer , Nathan J. Grin , Jonathan Mackey , Joachim M. Bestenlehner , Goetz Graefener

This paper discusses the location of a sample of planetary nebulae on the HR diagram. We determine the internal velocity fields of 14 planetary nebulae from high-resolution echelle spectroscopy, with the help of photoionization models. The…

Astrophysics · Physics 2008-11-26 Krzysztof Gesicki , Agnes Acker , Albert A. Zijlstra

We study the gas distribution and kinematics of the inner kpc of six moderately luminous (43.43$\leq$log$L_{\rm bol}\leq$44.83) nearby ($0.004 \leq z \leq 0.014$) Seyfert galaxies observed with the Near-infrared Integral Field Spectrograph…

We present high-dispersion spectroscopic data of the compact planetary nebula Vy 1-2, where high expansion velocities up to 100 km/s are found in the Ha, [N II] and [O III] emission lines. HST images reveal a bipolar structure. Vy 1-2…

Solar and Stellar Astrophysics · Physics 2016-08-08 S. Akras , P. Boumis , J. Meaburn , J. Alikakos , J. A. López , D. R. Gonçalves

Planetary nebulae (PNe) are strong H$\alpha$ line-emitters and a lot of new PNe discoveries have been made by the SuperCOSMOS AAO/UKST H$\alpha$ Survey (SHS) and the Isaac Newton Telescope Photometric H$\alpha$ Survey (IPHAS). However, the…

Solar and Stellar Astrophysics · Physics 2019-08-20 Stavros Akras , Lizette Guzman-Ramirez , Denise R. Gonçalves

We summarize new X-ray detections of four nitrogen-type Wolf-Rayet (WR) stars obtained in a limited survey aimed at establishing the X-ray properties of WN stars across their full range of spectral subtypes. None of the detected stars is so…

Solar and Stellar Astrophysics · Physics 2015-05-14 S. L. Skinner , S. A. Zhekov , M. Guedel , W. Schmutz , K. R. Sokal

We have carried out a spatial-kinematical study of three proto-planetary nebulae, IRAS 16594-4656, Hen 3-401, and Rob 22. High-resolution H2 images were obtained with NICMOS on the HST and high-resolution spectra were obtained with the…

Astrophysics · Physics 2009-11-13 Bruce J. Hrivnak , Nathan Smith , Kate Y. L. Su , Raghvendra Sahai

Ionized nebulae provide critical insights into the conditions of the interstellar medium (ISM). Their bright emission lines enable the measurement of physical properties, such as the gas-phase metallicity, across galaxy disks and in distant…

Extragalactic Planetary Nebulae (PNe) are not only useful as distance signposts or as tracers of the dark-matter content of their host galaxies, but constitute also good indicators of the main properties of their parent stellar populations.…

Cosmology and Nongalactic Astrophysics · Physics 2015-03-19 Marc Sarzi , Gary Mamon , Michele Cappellari , Eric Emsellem , Roland Bacon , Roger L. Davies , P. Tim de Zeeuw

The iconic planetary nebula (PN) NGC 7027 is bright, nearby (D ~ 1 kpc), highly ionized, intricately structured, and well observed. This nebula is hence an ideal case study for understanding PN shaping and evolution processes. Accordingly,…

Astrophysics of Galaxies · Physics 2023-01-04 Paula Moraga Baez , Joel H. Kastner , Bruce Balick , Rodolfo Montez , Jesse Bublitz

A detailed kinematic analysis of ionized gas in the nearby irregular galaxy NGC 4449 is presented. Observations are conducted in the spectral lines of Halpha and [SII]. Our scanning Fabry--Perot interferometric observations are presented…

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